Solar eclipse of September 10, 1923

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Solar eclipse of September 10, 1923
SE1923Sep10T.png
Map
Type of eclipse
Nature Total
Gamma 0.5149
Magnitude 1.043
Maximum eclipse
Duration 3m 37s
Coordinates 34.7N 121.8W
Max. width of band 167 km
Times (UTC)
Greatest eclipse 20:47:29
References
Saros 143 (18 of 72)
Catalog # (SE5000) 9335

A total solar eclipse occurred on September 10, 1923. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across the surface of the Earth, while a partial solar eclipse will be visible over a region thousands of kilometres wide.

The path of totality crossed the Pacific Ocean, northwestern and northern Mexico, Yucatan peninsula, Belize.

Related eclipses[edit]

Solar eclipses of 1921-1924[edit]

Each member in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the moon's orbit.

Solar eclipse series sets from 1921-1924
Ascending node   Descending node
118 April 8, 1921
SE1921Apr08A.png
Annular
123 October 1, 1921
SE1921Oct01T.png
Total
128 March 28, 1922
SE1922Mar28A.png
Annular
133 September 21, 1922
SE1922Sep21T.png
Total
138 March 17, 1923
SE1923Mar17A.png
Annular
143 September 10, 1923
SE1923Sep10T.png
Total
148 March 5, 1924
SE1924Mar05P.png
Partial
153 August 30, 1924
SE1924Aug30P.png
Partial

Solar 143[edit]

It is a part of Saros cycle 143, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on March 7, 1617 and total event from June 24, 1797 through October 24, 1995. It has hybrid eclipses from November 3, 2013 through December 6, 2067, and annular eclipses from December 16, 2085 through September 16, 2536. The series ends at member 72 as a partial eclipse on April 23, 2873. The longest duration of totality was 3 minutes, 50 seconds on August 19, 1887.[1]

Series members 17-28 occur between 1901 and 2100:

17 18 19
SE1905Aug30T.png
August 30, 1905
SE1923Sep10T.png
September 10, 1923
SE1941Sep21T.png
September 21, 1941
20 21 22
SE1959Oct02T.png
October 2, 1959
SE1977Oct12T.png
October 12, 1977
SE1995Oct24T.png
October 24, 1995
23 24 25
SE2013Nov03H.png
November 3, 2013
SE2031Nov14H.png
November 14, 2031
SE2049Nov25H.png
November 25, 2049
26 27 28
SE2067Dec06H.png
December 6, 2067
SE2085Dec16A.png
December 16, 2085

Notes[edit]

References[edit]